Showing posts with label cloud. Show all posts
Showing posts with label cloud. Show all posts

Wednesday, May 2, 2012

JCMT: The first detailed image of filamentary structure in Orion A cloud

The first detailed image of filamentary structure traced in the Northern part of the Orion A cloud, showing where the stars are forming from clumps of cold gas and dust. 

The ability to image condensations of cold dust with the earlier SCUBA camera, and more recently with SCUBA-2, has made the JCMT one of the choice instruments in the world for studying the earliest stages of star formation.

Credit: Johnstone et al.

Friday, January 6, 2012

UFO Cloud over the Crazy Mountains

A lenticular cloud, also called a UFO cloud, forms over the Crazy Mountains in Montana, USA

Picture: James Woodcock, Billings Gazette/AP

Wednesday, December 14, 2011

Disaster looms for gas cloud falling into Milky Way's central black hole

This view shows a simulation of how a gas cloud that has been observed approaching the supermassive black hole at the center of the galaxy may break apart over the next few years.

This is the first time ever that the approach of such a doomed cloud to a supermassive black hole has been observed and it is expected to break up completely during 2013.

The remains of the gas cloud are shown in red and yellow, with the cloud's orbit marked in red. The stars orbiting the black hole are also shown along with blue lines marking their orbits. This view simulates the expected positions of the stars and gas cloud in the year 2021. Credit: ESO/MPE/Marc Schartmann

The normally quiet neighbourhood around the massive black hole at the center of our Milky Way Galaxy is being invaded by a gas cloud that is destined in just a few years to be ripped, shredded and largely eaten.

Many, if not all, galaxies have massive black holes at their centers. But this supermassive black hole is the only one close enough for astronomers to study in detail, so the violent encounter is a unique chance to observe what until now has only been theorised: how a black hole gulps gas, dust and stars as it grows ever bigger.

"When we look at the black holes in the centers of other galaxies, we see them get bright and then fade, but we never know what is actually happening," said Eliot Quataert, a theoretical astrophysicist and University of California, Berkeley professor of astronomy.

"This is an unprecedented opportunity to obtain unique observations and insight into the processes that go on as gas falls into a black hole, heats up and emits light. It's a neat window onto a black hole that's actually capturing gas as it spirals in."

"The next two years will be very interesting and should provide us with extremely valuable information on the behaviour of matter around such massive objects, and its ultimate fate," said Reinhard Genzel, professor of physics at both UC Berkeley and the Max Planck Institute for Extraterrestrial Physics (MPE) in Garching, Germany.

The discovery by Genzel; Stefan Gillessen of the MPE; Quataert and colleagues from Germany, Chile and Illinois will be reported online Wednesday, Dec. 14, in advance of the Jan. 5 publication of the news in the British journal Nature.

Wednesday, August 17, 2011

Mystery of Titan's Bizarre Giant Cloud

A huge arrow-shaped storm blows across the equatorial region of Titan in this image from NASA's Cassini spacecraft, chronicling the seasonal weather changes on Saturn's largest moon. 

The part of the storm that is visible here measures 1,200 kilometers (750 miles) in length east-to-west and 1,500 kilometers (930 miles) in length.

CREDIT: NASA/JPL/SSI

The mystery of a giant arrow-shaped cloud on Saturn's largest moon Titan may now be solved, a new study suggests.

The enigma was likely caused by a massive wave rippling through the moon's atmosphere.

The discovery could help scientists better understand similar phenomena on Earth, especially in light of changing global climate, researchers said.

NASA's Cassini spacecraft detected the cloud at Titan's equator in September 2010. The cloud is huge, with each side running about 930 miles (1,500 kilometers) long.

Monday, June 6, 2011

Missing link found in the biology of cloud formation



Scientists have known for two decades that sulphur compounds that are produced by bacterioplankton as they consume decaying algae in the ocean cycle through two paths.

In one, a sulphur compound dimethylsulphide, or DMS, goes into the atmosphere, where it leads to water droplet formation - the basis of clouds that cool the Earth. In the other, a sulphur compound goes into the ocean's food web, where it is eaten and returned to seawater.

What they haven't known is how sulphur is routed one way or the other or why.

They also have wondered what if - in a time of growing concern about global warming - it was possible to divert the sulphur compound that goes into the oceans into the atmosphere, helping to mitigate global warming?

A study by researchers at the University of Georgia just published in Nature brings the possibility of using the sulphur cycle to mitigate global warming closer with the identification of the steps in the biochemical pathway that controls how bacteria release the sulphur compound methanethiol, or MeSH, into the microbial food web in the oceans and the genes responsible for that process.

"With our increased understanding of the sulphur cycle in the ocean," said study co-author William (Barny) Whitman, "we are now better able to evaluate the impacts of climate change on the process and the potential for its manipulation, which has been proposed as a way to mitigate global warming.

"It's wonderful to have this much understanding of a major biogeochemical process," noted Whitman, distinguished research professor and head of the department of microbiology in the Franklin College of Arts and Sciences.

In addition to elucidating the steps in the pathway and identifying the responsible genes, the team of UGA microbiologists, marine scientists and chemists discovered that the pathway is found widely, not only among bacterioplankton in the ocean but also in non-marine environments.

"The big mystery about bacteria is what they are doing in nature," Whitman said. "The organisms metabolise compounds for their own needs. We need to understand what they are getting out of it to understand what it means for the ocean, and now it will be possible to look at the environmental importance of this process and how it's regulated." That will help to answer the "why" of the two sulphur fates.

Co-authors of the Nature paper were UGA graduate students Chris Reisch and Vanessa Varaljay, department of microbiology; graduate student Melissa Stoudemayer and Jon Amster, professor and head, department of chemistry; and distinguished research professor Mary Ann Moran, department of marine sciences-all in the Franklin College of Arts and Sciences.

The collaborators in this study built on a line of research begun at UGA over a decade ago. Moran's early research showed that an abundant group of bacteria known as marine roseobacters play a role in moving dimethylsulphonioproprionate (DMSP), the chemical made by marine algae and released into the water upon their death, into the atmosphere as the compound dimethylsulphide (DMS).

Missing link found in the biology of cloud formation over the oceans

Tuesday, September 14, 2010

Suspended disbelief:The Boy in the Bubble

Balloons 2

The Boy in the Bubble and the Girl holding the strings!

"My favourite photograph features my daughter holding some helium balloons and I am standing on them in mid air. It was lovely working with my daughter and the photo represents my feelings," he said

Picture: Li Wei/Solent News & Photo Agency